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- W2076537573 abstract "H I Lyα spectral line profiles have been measured in polar regions of the solar corona at projected heliocentric heights of 1.8-3.5 R☉. Observations were made with the Ultraviolet Coronal Spectrometer on the Spartan 201 satellite from 16:52 to 04:04 UT on 1993 April 11-12 (south pole) and from 12:28 to 22:09 UT on 1993 April 12 (north pole). In general, the coronal profiles cannot be accurately curve-fitted with a single-Gaussian function. The fits with two Gaussians yield most probable velocities of 158 and 322 km s-1 (south) and 98 and 266 km s-1 (north). These parameters vary by less than 10% (1 σ) over the observed heights." @default.
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- W2076537573 date "1996-07-10" @default.
- W2076537573 modified "2023-10-15" @default.
- W2076537573 title "Measurement of Hydrogen Velocity Distributions in the Extended Solar Corona" @default.
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- W2076537573 doi "https://doi.org/10.1086/310145" @default.
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